Efficient neutrino production requires an external radiation field stronger than the magnetic field near the broad-line region, but this conflicts with single-zone broadband emission, implying the neutrino site must be physically separated from the dominant electromagnetic zone in uncommon jet confi
The Contribution of Fermi-2LAC Blazars to Diffuse TeV-PeV Neutrino Flux
4 Pith papers cite this work. Polarity classification is still indexing.
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SKA-VLBI can deliver high-sensitivity milliarcsecond imaging and polarimetry of faint blazars to constrain models of high-energy photon and neutrino emission in AGN jets.
Calibrated AGN disk-wind models contribute ≲5% to the CGB above 10 GeV and ≲10% to the CNB at 100 TeV and are unlikely to dominate either background.
Review assessing HSP BL Lacs as UHECR and neutrino sources, noting strains from baryonic loading, heavy-nuclei preference in Auger data, and isotropy mismatch with beamed sources.
citing papers explorer
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Locating the Production Sites of High-Energy Neutrinos in Blazar Jets
Efficient neutrino production requires an external radiation field stronger than the magnetic field near the broad-line region, but this conflicts with single-zone broadband emission, implying the neutrino site must be physically separated from the dominant electromagnetic zone in uncommon jet confi
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SKA-VLBI Probes of High-energy Emission Processes in Relativistic Jets
SKA-VLBI can deliver high-sensitivity milliarcsecond imaging and polarimetry of faint blazars to constrain models of high-energy photon and neutrino emission in AGN jets.
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Revisiting Disk Winds in Active Galactic Nuclei as an Origin of Cosmic Gamma-ray and Neutrino Backgrounds
Calibrated AGN disk-wind models contribute ≲5% to the CGB above 10 GeV and ≲10% to the CNB at 100 TeV and are unlikely to dominate either background.
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High-Synchrotron-Peaked BL Lacs as Multi-Messenger Sources: Connecting Ultra-High-Energy Cosmic Rays and Neutrinos
Review assessing HSP BL Lacs as UHECR and neutrino sources, noting strains from baryonic loading, heavy-nuclei preference in Auger data, and isotropy mismatch with beamed sources.